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Titlebook: Galactic Astrophysics and Gamma-Ray Astronomy; Proceedings of a Mee G. E. Morfill,R. Buccheri Conference proceedings 1983 D. Reidel Publish

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發(fā)表于 2025-3-21 17:54:24 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書(shū)目名稱(chēng)Galactic Astrophysics and Gamma-Ray Astronomy
副標(biāo)題Proceedings of a Mee
編輯G. E. Morfill,R. Buccheri
視頻videohttp://file.papertrans.cn/381/380328/380328.mp4
圖書(shū)封面Titlebook: Galactic Astrophysics and Gamma-Ray Astronomy; Proceedings of a Mee G. E. Morfill,R. Buccheri Conference proceedings 1983 D. Reidel Publish
描述This book contains the invited and contributed lectures presented at a meeting organised in the context of the XVIII general assembly ofthe IAU, held in Patras, August 19, 1982. Roughly one hundred scientists attended this meeting, the discussions were livel- sometimes heated - and the original time span allocated to the meeting was as a result, comfortably exceeded by about 50 % . The aim of this meeting was to determine the role of galactic gamma-ray astronomy within the general concept of galactic astrophysics. The timing, at the end of the COS-B mission, was regarded as opportune, because it gives interested astrophysicists the possibility for interdisciplinary studies using the existing gamma-ray data base (e.g. comparison with infrared, radio, X-ray, etc. astronomies), as well as for theoretical studies. The next generation of gamma-ray detectors will probably not be in operation for another 5 to 10 years, and therefore it is hoped that the proceeding of this meeting can be used (in the intermediate time) as a basis for further studies, as a stimulation for more theoretical work and as an important contribution for defining the aims and operation of future gamma-ray missions.
出版日期Conference proceedings 1983
關(guān)鍵詞Galaxy; Supernova; astronomy; astrophysics; cosmic ray; galaxies; gamma-ray burst; stellar
版次1
doihttps://doi.org/10.1007/978-94-009-7208-7
isbn_softcover978-94-009-7210-0
isbn_ebook978-94-009-7208-7
copyrightD. Reidel Publishing Company, Dordrecht, Holland 1983
The information of publication is updating

書(shū)目名稱(chēng)Galactic Astrophysics and Gamma-Ray Astronomy影響因子(影響力)




書(shū)目名稱(chēng)Galactic Astrophysics and Gamma-Ray Astronomy影響因子(影響力)學(xué)科排名




書(shū)目名稱(chēng)Galactic Astrophysics and Gamma-Ray Astronomy網(wǎng)絡(luò)公開(kāi)度




書(shū)目名稱(chēng)Galactic Astrophysics and Gamma-Ray Astronomy網(wǎng)絡(luò)公開(kāi)度學(xué)科排名




書(shū)目名稱(chēng)Galactic Astrophysics and Gamma-Ray Astronomy被引頻次




書(shū)目名稱(chēng)Galactic Astrophysics and Gamma-Ray Astronomy被引頻次學(xué)科排名




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書(shū)目名稱(chēng)Galactic Astrophysics and Gamma-Ray Astronomy讀者反饋




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發(fā)表于 2025-3-21 23:44:47 | 只看該作者
Kathy Lee-Son,Massimo Attanasio in Patras, August 19, 1982. Roughly one hundred scientists attended this meeting, the discussions were lively — sometimes heated — and the original time span allocated to the meeting was a result, comfortably exceeded by about 50%.
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https://doi.org/10.1007/978-1-4613-4024-9ow component might result from the interaction between cosmic rays and H. gas. The mass of gas in the Galactic Center is not large enough to produce the gamma-ray peak, but enough to produce the far-infrared peak. The relation of far-infrared dip and near-infrared hump near . = 356° to gamma-ray hump is discussed.
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發(fā)表于 2025-3-22 14:42:49 | 只看該作者
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發(fā)表于 2025-3-22 17:19:08 | 只看該作者
Cosmic Gamma Rays and Molecular Gas in the Galaxy,It is shown that, locally, γ-ray data enable the calibration of H. densities to be inferred from CO data and elsewhere the variation of cosmic-ray intensity with position to be assessed. Finally, the importance of cosmic-ray irradiated molecular clouds in simulating γ-ray ‘sources’ is reiterated.
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發(fā)表于 2025-3-22 23:31:44 | 只看該作者
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發(fā)表于 2025-3-23 02:42:44 | 只看該作者
Comparison of Far-Infrared Radiation with Gamma Radiation,ow component might result from the interaction between cosmic rays and H. gas. The mass of gas in the Galactic Center is not large enough to produce the gamma-ray peak, but enough to produce the far-infrared peak. The relation of far-infrared dip and near-infrared hump near . = 356° to gamma-ray hump is discussed.
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發(fā)表于 2025-3-23 09:26:40 | 只看該作者
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